The space age has finally begun.

The United States and its allies, including China, Russia, India, Japan and others, are planning to use the Hubble’s successor, the James Webb Space Telescope, to study the universe.

And now, a team of astronomers is trying to figure out what they might see.

Led by astrophysicist Stephen Hawking and MIT professor Brian Cox, the group recently presented a paper describing the new James Webb telescope in a conference in San Diego.

The telescope is being developed by the Space Telescope Science Institute (STScI) and the Jet Propulsion Laboratory, which is headed by retired NASA director Jim Green.

The STScI team includes scientists from Harvard University, Caltech, Harvard University’s James Webb Center for Space Studies and the University of Texas at Austin.

Their work was published online last week in the journal Science Advances.

The paper focuses on two aspects of the telescope: how to design a small telescope, and how to find a suitable environment for observing the cosmic microwave background (CMB), a light signal that appears as a faint echo of a star’s light.

The CMB, which was first detected in the early 1980s, was originally detected with the Hubble telescope.

Its brightness depends on the temperature of the universe, but scientists say its most important measurement is the age of the Universe.

This is due to the fact that the universe is billions of years old.

As the universe ages, it emits a steady stream of cosmic rays that are scattered in the universe’s microwave radiation, which can be seen with the naked eye.

These cosmic rays are then absorbed by matter in the Universe, and become more and more dim over time.

By measuring the energy of these cosmic rays and the CMB light they emit, scientists can measure how the Universe was formed.

The team was able to use data from the CGB to estimate the age and composition of the cosmos, and also measure the composition of various kinds of matter, including stars, planets and asteroids.

The researchers also used these data to estimate how much mass there is in the cosmos.

As they discovered that the Universe is about 7.6 billion years old, the team calculated that there are about 2.4 billion atoms in the whole universe.

This amount is similar to the amount of mass of the Sun, which contains about 10.5 billion atoms.

The astronomers were also able to determine that the CIB has about a 1 percent chance of having the same mass as the Sun.

They found that the mass of an atom in the CUBE is about one millionth that of the mass in the Sun and a few hundredths that of all the known stars in the Milky Way.

That means that the Sun’s mass is about 1.7 times more massive than the mass we find in the Cosmic Microwave Background (CBM), which was discovered by NASA’s Hubble Space Observatory in 2003.

This indicates that our Sun has about 50 times more mass than the Sun would have if it had formed in a star-like state, such as the Cumbrian supernova explosion known as a supernova.

In a separate paper, the researchers also determined that about 40 percent of the CMRBs in the sky are located in galaxies known as spiral arms, which are galaxies that are rotating very slowly and very rapidly.

These are objects that are spinning faster than the speed of light.

When you look at a spiral galaxy, you see that they have a big amount of material coming from the center, which has a lot of mass coming from outside.

This material is being pushed out by the spinning spiral arms.

This is where the scientists were able to calculate that about 80 percent of CMBs in the galaxy were found in spiral arms with a mass about 1 million times that of our Sun.

This means that about 60 percent of all CMB’s are likely in spiral galaxies with a total mass about one billion times the mass our Sun, and 40 percent are in galaxies with masses much lower than our Sun’s.

According to the authors, this means that we can use the new data to infer whether there are any stars that could be found in galaxies that have such large masses.

The scientists also noted that the new paper does not directly address whether there might be galaxies with even more mass.

The reason that they used the CMM for this study was to study other astrophysical phenomena, like the cosmic inflation that took place in the mid-1990s and which led to the formation of the Large and Small Magellanic Clouds, as well as the gravitational lensing of galaxies.

However, this study does suggest that if we can find more stars in galaxies like the ones in the Hubble study, we could eventually be able to find some stars in these galaxies.

If we can confirm this in the next few years, it would give us more evidence for the existence of supermassive black holes in the galactic